Photometric observations of eight C class and 1 S class
asteroids are presented. Light curve fragments determined in
this study will be used with future observations to
determine rotation rates of observed asteroids. This is part
of an ongoing survey to photometrically observe primitive
asteroids as a precursor to observing the same asteroids
spectroscopically. Spectroscopic observations will be used
to search for evidence of aqueous alteration on the asteroid
surface. Photometry results will enhance this by
establishing rotation periods, pole orientation, and shape;
hence, a better understanding of where on the surface the
alteration has taken place.